5XMM J064041.3+094809
5XMM-DR15 stacked source · SRCID 3001142010100122
Position:
06h40m41.38s +09d48m09.2s
(100.17242°, 9.80255°)
EP flux
2.23e-14
± 2.1e-15
erg cm-2 s-1
CLASSX
Star
(0.974)
Detections
1
| SRCID | 3001142010100122 |
|---|---|
| IAUNAME | 5XMM J064041.3+094809 |
| SC_RA | 06h40m41.38s (100.17242°) |
| SC_DEC | +09d48m09.2s (9.80255°) |
| RADEC_ERR | 0.41 arcsec |
| LII / BII | 202.9869° / 2.0928° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 51988.103 (2001-03-20 02:28:07.000 UTC) |
| MJD_LAST | 51988.575 (2001-03-20 13:48:05.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.23e-14 ± 2.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.61
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.22
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.07
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.39e-14 (+3.6e-14 / −3.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.64e+21 (+1.8e+21 / −1.4e+21) cm−2 |
| Photon index (Γ) | 2.96 (+2.99 / −2.91) |
| DoF | 704 |
| p-value | 0.004 |
| Inter-instrument norm. | 0.84 (0.75–0.96) |
| Quality flag | 7 |
| APPROX_SOURCE_VAR | 5.700 (approximate flux variability amplitude) |
|---|
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.